Baade’s window direction: kinematics. All DIB velocities are found to be consistent with the local HI, around 5 km s^-1. The second velocity component allowed by the fitting procedure is found to be unnecessary or negligible. Note that the discrepant data point at +15 km s^-1 for the 6283 Å DIB (lower panel) is due to the effect of a strongly discrepant stellar line and disappears when the fitting is repeated after masking the corresponding region (the total EW is found to be unchanged).